Nuclear astrophysics with intermediate-energy RI beams

Details Nuclear astrophysics with intermediate-energy RI beams Nuclear astrophysics with intermediate-energy RI beams

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..425..362m&link_type=abstract

Tours symposium on nuclear physics III. AIP Conference Proceedings, Volume 425, pp. 362-371 (1998).

Physics

Nuclear Physics

1

Coulomb Excitation, Transfer Reactions, Charge-Exchange Reactions, Hydrostatic Stellar Nucleosynthesis

Scientific paper

Recent development of RI beam production opens a new possibility of research in nuclear astrophysics. At intermediate-energies (several tens to several hundreds MeV/u), thermonuclear reactions can be studied indirectly by the Coulomb dissociation and Coulomb excitation reactions, and possibly also by the transfer and charge-exchange reactions with inverse kinematics. A brief review and perspectives for studies using these reactions are given.

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